The fastest CME is found from an interval of time, and propagated to Earth, in two steps, first to obtain the Solar wind speed at Earth and then propagated again with a more reasonable CME speed.
The output produces Min-Max ETAs for each object in the heliosphere and the plots of the final propagation model.
This Workflow was produced as one of the challenges in the HELIO CDAW-IV hosted at TCD

This workflow takes a single VOTable and splits it up in a vector for the names of fields, a vector for the UCDs of the fields, a vector for the UTypes of the fields, and a two dimensional vector for the values.

Run the cir backwards propagation code on the HELIO processing service.
Required inputs: time start of backwards propagation, the object (planet/spacecraft) from where the propagation should start, assumed solar wind speed at the time, assumed error of solar wind speed
Output: VOTable with times at different points in solar system